STUDY OF PRASEODYMIUM STRONTIUM MANGANITE FOR THE POTENTIAL by

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STUDY OF PRASEODYMIUM STRONTIUM MANGANITE FOR THE POTENTIAL
USE AS A SOLID OXIDE FUEL CELL CATHODE
by
Matthew Edward Pfluge
A thesis submitted in partial fulfillment
of the requirements for the degree
of
Master of Science
in
Chemical Engineering
MONTANA STATE UNIVERSITY
Bozeman, Montana
April 2005
©COPYRIGHT
by
Matthew Edward Pfluge
2005
All Rights Reserved
ii
APPROVAL
of a thesis submitted by
Matthew Edward Pfluge
This thesis has been read by each member of the thesis committee and has been
found to be satisfactory regarding content, English usage, format, citations,
bibliographical style, and consistency, and is ready for submission to the College of
Graduate Studies.
Dr. Max Deibert
Approved for the Department of Chemical Engineering
Dr. Ron Larsen
Approved for the College of Graduate Studies
Dr. Bruce McLeod
iii
STATEMENT OF PERMISSION TO USE
In presenting this thesis in partial fulfillment of the requirements for a master’s
degree at Montana State University, I agree that the Library shall make it available to
borrowers under the rules of the Library.
If I have indicated my intention to copyright this thesis by including a
copyright notice page, copying is allowable only for scholarly purposes, consistent with
“fair use” as prescribed in the U.S. Copyright Law. Requests for permission for extended
quotation from or reproduction of this thesis in whole or in parts may be granted only by
the copyright holder.
Matthew Edward Pfluge
April 14, 2005
iv
ACKNOWLEDGEMENTS
I would like to personally thank all of the researchers at Pacific Northwest
National Lab that helped me through my journey especially Greg Coffey, Pete Rieke,
Larry Pedersen, Ed Thomsen, Carolyn Nguyen, Kerry Meinhardt, Steve Simner, Mike
Anderson, and Doug Conner. I would also like to thank my advisors, Dr. Max Deibert
and Dr. Dick Smith for their support and always challenging me. I would also like to
acknowledge the organizations that provided funding and made this possible including
PNNL, SECA, DOE, and specifically the Office of Fossil Energy Advanced Research
and Technology Development Materials Program. Finally, I would like to thank my
family for their love and support, and Michelle for keeping me going.
v
TABLE OF CONTENTS
1. INTRODUCTION ......................................................................................................... 1
2. BACKGROUND AND LITERATURE REVIEW ....................................................... 2
Solid Oxide Fuel Cells (SOFC) ....................................................................................... 2
SOFC Basics .............................................................................................................. 2
Decreasing SOFC Operating Temperature ................................................................ 5
SOFC Cathode............................................................................................................ 7
Mixed Conductor Theory and Modeling ......................................................................... 8
Perovskite Structure ................................................................................................... 8
“A” Site Deficiency Importance .............................................................................. 10
Influence of Doping ................................................................................................. 11
Relevant Cathode Systems ............................................................................................ 12
LaSrMnO3 ................................................................................................................ 12
PrSrMnO3 ................................................................................................................. 14
3. EXPERIMENTAL PROCEDURES............................................................................ 17
Glycine-Nitrate Pyrolosis .............................................................................................. 17
Sample Preparation........................................................................................................ 20
Calcination ............................................................................................................... 20
Attrition Milling ....................................................................................................... 20
Ink Preparation ......................................................................................................... 21
Pellet and Bar Pressing............................................................................................. 21
XRD Evaluation ............................................................................................................ 22
Phase Purity.............................................................................................................. 22
Archimedes Density ................................................................................................. 23
Dilatometry.................................................................................................................... 23
Electronic Conductivity................................................................................................. 24
Ionic Conductivity ......................................................................................................... 25
Seebeck Measurements.................................................................................................. 26
Half – Cell Measurements ............................................................................................. 27
4. RESULTS AND DISCUSSION .................................................................................. 29
XRD Evaluation ............................................................................................................ 29
Phase Purity Peaks ................................................................................................... 29
Relative Density ....................................................................................................... 31
Dilatometry.................................................................................................................... 32
Sintering Study......................................................................................................... 32
TEC Calculation....................................................................................................... 33
Analysis.................................................................................................................... 34
vi
TABLE OF CONTENTS CONTINUED
Electronic Conductivity................................................................................................. 35
Calculations.............................................................................................................. 35
Analysis.................................................................................................................... 38
Ionic Conductivity ......................................................................................................... 39
Calculations.............................................................................................................. 39
Analysis.................................................................................................................... 40
Seebeck Measurements.................................................................................................. 41
Calculations.............................................................................................................. 41
Analysis.................................................................................................................... 42
Half – Cell Measurements ............................................................................................. 43
Calculations.............................................................................................................. 43
Analysis.................................................................................................................... 52
5. CONCLUSIONS AND RECOMMENDATIONS ...................................................... 54
SOURCES CITED............................................................................................................ 56
vii
LIST OF TABLES
Table
Page
1: PSM compositions and nitrate solutions for glycine-nitrate combustion. ...................18
2: Sample mass calculations for nitrate solution and glycine. .........................................19
3: Relative and percent densities calculations .................................................................31
4: Tabulated values of chemical reaction constants and area specific resistance
throughout the cathode layer......................................................................................46
viii
LIST OF FIGURES
Figure
Page
2.1 Schematic of Solid Oxide Fuel Cell [4]........................................................................4
2.2 ABO3 perovskite structure. .........................................................................................10
3.1 Sample used for the four-point AC conductivity experiments. ..................................24
3.2 Oxygen permeation assembly. ....................................................................................25
3.3 Assembly structure for Seebeck coefficient measurements........................................26
3.4 Half-cell measurement set-up. ....................................................................................27
4.1 XRD phase peaks for the PSM data set with references for silicon, PSM and
Hausmannite. .............................................................................................................30
4.2 Densification Study of samples up to 1400oC. ...........................................................33
4.3 TEC measurements of sample set with comparison to common electrolyte and anode
material. .....................................................................................................................34
4.4 Electrical conductivity measurement from 200oC to 950oC. ......................................36
4.5 Arrenhius plot of electrical conductivity measurement. .............................................37
4.6 Activation energies for electrical conductivity. ..........................................................38
4.7 Oxygen permeation from 200oC to 950oC. .................................................................40
4.8 Seebeck measurements for the sample set from 100oC to 950oC. ..............................41
4.9 Half cell measurement for sample set at 850oC in air.................................................44
4.10 Example of hyperbolic sine curve fit to PSM 10 data at 850oC. ..............................45
4.11 PSM 10 half cell after testing....................................................................................47
4.12 PSM 20 half cell after testing....................................................................................48
4.13 PSM 20A half cell after testing.................................................................................49
4.14 PSM 30 half cell after testing....................................................................................50
4.15 PSM 30A half cell after testing.................................................................................51
ix
ABSTRACT
Extensive research has been performed on solid oxide fuel cell cathodes. These
cathodes must be stable in the oxidation environment and have sufficient electrical
conductivity and catalytic activity for the oxidant gas reaction at the appropriate
operating temperature. Also, the cathode must be chemically and thermally compatible
with the other cell components at room temperature, operating temperatures, and higher
fabrication temperatures. Praseodymium strontium manganite (PSM) has shown
promising electrical properties with respect to ideal properties of cathodes in solid oxide
fuel cells. Various dopant levels of strontium in the perovskite structure were
investigated, which include Pr1-xSrxMnO3-δ where x = 0.10, 0.20, 0.30 and (Pr1xSrx)0.98MnO3-δ where x = 0.20 and 0.30. This cathodic material has shown electrical
conductivity over twice as high as a traditionally used cathode, La0.8Sr0.2MnO3. Through
this investigation, the electrical and ionic conductivities of this ceramic series were
measured from 200oC to 950oC. Another important electrical measurement investigated
was the Seebeck coefficient within the same temperature range. This coefficient is a
measurement of the change in voltage across a temperature gradient and thus can be
referred to as its thermal power. Conductor types have been interpolated from the
measurements. This measurement provides an improved understanding of the high
electrical properties displayed within the material. Cathodic overpotential was also
measured using half cell reactions performed in the temperature range of 650oC to 850oC
under both air and pure oxygen. This measurement was used to calculate the current
exchange density of the cathode and the area specific resistance. Overall, as the
strontium concentration increased, the electrical activity of the ceramic subsequently
increased. Furthermore, in relation to the traditional cathode material, La0.8Sr0.2MnO3,
the substitution of lanthanum with praseodymium has produced more effective cathodic
performance.
1
CHAPTER 1
INTRODUCTION
Solid oxide fuel cells (SOFC) have been studied extensively for a broad spectrum
of electrical power generation applications because of their clean and efficient electrical
energy production. The potential for these fuel cells is immense and they promise to be
an important alternative energy source for a less oil dependant future.
Technological developments of this promising energy source are in their
developmental stage with copious challenges left to be resolved before the SOFC fuel
cell can be fully utilized. SOFC technology has recently received vast amounts of
funding originating from the Department of Energy resulting in advances in ceramic
technology, engineering material compositions, testing methods, property relationships,
and processing intricate matrices. Additionally, this research, conducted through the
Department of Energy, has sparked further advances in ceramic synthesis,
characterization, and other properties.
2
CHAPTER 2
BACKGROUND AND LITERATURE REVIEW
Solid Oxide Fuel Cells (SOFC)
SOFC Basics
Solid oxide fuel cells are prominent candidates for power generation that convert
chemical energy directly to electricity with high efficiency and little pollution. This
device bypasses the conversion of the chemical energy of the fuel into thermal and
mechanical energy which leads to losses and therefore achieves a theoretical efficiency
significantly higher than that of conventional power generation methods. This efficiency
is around 45% to 60% and may achieve an even higher efficiency if the byproduct heat is
fully utilized in the system [1].
Fuel cells have many advantages over conventional power generators. Fuel cells
are more versatile than conventional mechanical power generation devices, and they can
be increased and decreased in size for a variety of applications relevant to different power
needs [2]. Furthermore, the efficiency of the fuel cell is independent of size and can be
designed to follow loads with fast response times.
The fuel cell’s operation is, in
addition, quiet because of the lack of moving parts; therefore, fuel cells can be located
anywhere, including within residential areas. Another advantage of fuel cells is the fact
that they are environmentally friendly devices, especially considering fuel cells are
3
capable of using a variety of different fuels with minute environmental impacts.
Emissions of pollutants like NOx, SOx, and dangerous particulates from fuel cells are far
lower than those from conventional power generators [1]. Certain high temperature fuel
cells like SOFCs also have a multifuel capability. Since these fuels cells are operated at
an elevated temperature, they can process hydrocarbon fuels internally through reforming
reactions and do not need expensive subsystems to process these fuels.
It is this
particular capability of the fuel cell that will likely facilitate a transition from
conventional fuel sources like gasoline and natural gas to strictly hydrogen gas [1].
The main distinction among ceramic fuel cells is a solid ceramic material that
conducts ions without electrical conduction called the electrolyte with two ceramic
electrodes attached on either side of this electrolyte, one being the cathode while the
other is the anode. The ionic permeation requirement through this ceramic electrolyte
necessitates a high operating temperature from 600oC to 1000oC [3]. These intense
temperatures promote rapid reaction kinetics, allow reforming of hydrocarbon fuels, and
generate byproduct heat.
However, stringent material restrictions and processing
requirements required by these extreme temperatures prove to be a disadvantage of
SOFCs.
A schematic of a solid oxide fuel cell is shown in figure 2.1.
4
Figure 2.1: Schematic of Solid Oxide Fuel Cell [4].
A solid oxide fuel cell consists of a solid ceramic electrolyte surrounded by two ceramic
electrodes: a cathode and an anode. Fuel is fed on the anode side and undergoes an
oxidation reaction while releasing electrons to an external circuit. Air or pure oxygen is
fed to the cathode side where it undergoes a reduction reaction and accepts the electrons
from the circuit.
This electron flow produces direct current electricity.
The solid
electrolyte conducts oxygen ions from the cathode to the anode to complete the
electrochemical process. If methane is fed to the anode side, it is steam reformed by:
CH4 + H2O = CO + 3H2
The reactions on the anode side are:
H2 + O2- = H2O + 2e- ; CO + O2- = CO2 + 2e-
5
The reaction on the cathode side is:
½ O2 + 2e- = O2Therefore, the overall reactions for the fuel cell are:
H2 + ½ O2 = H2O; CO + ½ O2 = CO2
Therefore, the SOFC is considered to be an oxygen dilution cell, so the reversible open
circuit voltage for the fuel cell is given by the Nernst equation [1]:
Er
R⋅ T
4⋅ F
⎛ PO2( c) ⎞
⋅ ln⎜
⎝ PO2( a) ⎠
where R is the gas constant, T the temperature, F the Faraday’s constant, and PO2 the
partial pressure of oxygen at the electrode. The overall cell voltage can be described by:
V
Er − iR − η a − η c
where iR is the ohmic resistance, ηa, ηc are the anode and cathode polarizations [5].
Decreasing SOFC Operating Temperature
Currently, the operating temperature of a solid oxide fuel cell is around 1000oC;
however, many limitations occur at such a high temperature. Chemical instabilities
among different cell components develop, along with the diffusion of different elements
throughout the ceramic matrix from individual components into adjacent components [6].
Porous ceramic electrodes densify at these high operating temperatures, which decreases
the oxygen flux on the cathode side and the flux of fuel gas on the anode side toward the
electrolyte. This drastically decreases the overall performance of the fuel cell [7]. Also,
the individual cell components experience delamination due to slight differences in the
6
thermal expansion coefficient and the extreme thermal cycling experienced by the fuel
cell. Finally, the largest limitation of high operating temperatures is the fact that the
interconnect and manifolding materials required at these temperatures become the most
expensive components of the fuel cell [1].
Considering all of the disadvantages of the high operating temperature, it is
evident that research is needed in order to decrease the temperature to 650oC to 750oC
[5]. With such an alteration in temperature, the lifetime of the fuel cell is greatly
increased due to decreased interactions of the electrodes and the electrolyte. Ferritic
stainless steels can be used for the interconnect material, which are less expensive raw
materials and have lower manufacturing costs than the traditional ceramic lanthanum
strontium chromite interconnect. The manifolding material is also less costly. Also, the
startup time for the SOFC is significantly less [1].
With all of the advantages of decreasing the operating temperatures, the transition
seems to be inevitable; however, many challenges must be overcome.
Oxygen
permeation and electrical conductivities are thermally activated and significantly increase
with rising temperatures.
Oxygen ionic conductivity through the electrolyte
exponentially decreases, increasing the overall cell resistance. An additional source of
performance loss is in the charge transfer polarization of electrodes. To combat these
challenges, the electrodes need to have a higher electrical and ionic conductivity.
Furthermore, these electrodes need to have a fine grain size and higher porosity to
increase the number of sites for charge transfer reactions. All components need to be
manufactured thinner to decrease the ohmic resistance throughout the fuel cell [1-7].
7
SOFC Cathode
The main function of the cathode is to provide reaction sites for the
electrochemical reduction of the oxidant, O2. The cathode must be stable in the oxidation
environment and have sufficient electrical conductivity and catalytic activity for the
oxidant gas reaction at the appropriate operating temperature. Also, the cathode must be
chemically and thermally compatible with the other cell components from room
temperature to the operating temperature and to even higher fabrication temperatures [8].
The cathode has to be chemically, morphologically, and dimensionally stable in
an oxidant environment. It can not have disruptive phase transformations throughout the
temperature range from room temperature to the operating temperature. In addition, the
desired microstructure must be maintained in long-term operation because significant
changes can degrade the performance of the fuel cell [1].
Electrical conductivity of the cathode must support significant electron flow to
the reaction sites at the interface of the electrolyte and cathode in the oxidizing
environment at the operating temperature.
Maximum conductivity correlates to a
minimization of ohmic losses throughout the fuel cell. Ionic conductivity of the cathode
is important as well. The ability of the cathode to conduct oxygen ions provides more
oxygen sites to the electrolyte interface, which will improve the overall performance of
the fuel cell.
Compatibility of the cathode with other components is another important aspect
of its development. Chemical reactions and elemental interdiffusion between the cathode
and adjoining components needs to be limited or completely eliminated to minimize
8
second phase formations, stability reduction, change in thermal expansion, enhanced
electrical conductivity of the electrolyte and elimination of ionic conductivity in the
electrolyte among other effects [1].
The thermal expansion coefficient of the cathode needs to match all other cell
components from room temperature to the operating temperatures.
This will avoid
cracking and delamination during fabrication and operating with thermal cycling.
The cathode needs to have sufficient porosity to allow oxidant gas transport to the
reaction sites near the cathode-electrolyte interface. The lower limit on porosity is based
on the mass transport of the oxidant gas, while the upper limit is based on mechanical
strength of the component. There needs to be sufficient contact area of the cathode to the
electrolyte to provide enough reaction sites and enough porosity to supply sufficient
oxidant gas transport.
A combination of these essential requirements should correlate to the catalytic
activity of the cathode. Other desirable properties are high strength and toughness, ease
of fabrication, and ultimately a low cost. Electronic or mixed conducting oxides are the
best suited for the cathodic duties.
Mixed Conductor Theory and Modeling
Perovskite Structure
Most mixed conducting ceramic materials have the most desirable properties for a
SOFC while in the perovskite structure.
This structure is named from the mineral
9
perovskite, which has a chemical formula of CaTiO3 and is a naturally occurring mineral
that is abundant in chlorite, talc, and serpentine rocks. However, in this case, the term
perovskite refers to the ABO3 structure that is used for a wide variety of mixed conductor
systems. The ABO3 perovskite structure has technological applications that make use of
this structure’s ability to form oxygen vacancies with proper amounts of doping ions with
differing oxidation states. This is due to perovskites having large tolerances for departure
from ideal stoichiometry [3].
The principal perovskite structure is cubic containing three distinct sites for ions:
A, B, and O, shown in figure 2.2. The A and B atoms represent cations, while the O
refers to the oxygen anion with a negative 2 charge. In general terms, the ABO3 structure
can be described as face-centered cubic with A atoms at the corners, O atoms on the
faces, and a B atom occupying the octahedral site in the center. The largest of the cations
is the A site cation.
10
A site
B site
Oxygen
Figure 2.1: ABO3 perovskite structure.
“A” Site Deficiency Importance
In figure 2.2, a typical perovskite structure is shown. Using Pr and Sr as A site
atoms and Mn as the B site atom, the A site atoms, especially Pr atoms, are larger than
the Mn atoms in the B site. This means that the A site atoms dominate the overall
crystalline structure. Considering perovskite structure consisting of more A site atoms
than B site, the larger A site atoms will expand the crystalline structure in the direction of
the Pr atoms, which will deform and construe the structure creating a non-cubic or nonideal structure. In order to eliminate this phenomenon, a B site rich or A site deficient
structure is created. Therefore, the effects of a 2% A site deficiency were studied.
11
Influence of Doping
The ability of the perovskite structure to tolerate changes in its stoichiometry
means that the material can be altered by the substitution of different cations in the A and
B sites. Several functional properties of a perovskite can be modified by the total or
partial replacement of the A and B site cations. Since mixed conductors are candidates
for structures that require large amounts of ionic conductivity, one of the more frequent
reasons for doping a material with ions with differing oxidation states is to increase the
ionic conductivity.
One of the most common methods of doing this is an A-site
substitution to facilitate the formation of oxygen vacancies [3].
Transition metals are normally used for the B site atoms as they can assume a
mixed-valence state. The partial substitution of the A site cations by other metal cations
with lower valence states can cause the formation of oxygen vacancies.
This is
accompanied by a decrease in the B site cation valence states. This allows the material to
maintain charge neutrality [10]:
[A ] = [B ]+ [V ]
'
A
•
B
••
O
where AA' refers to doping the A site with a cation with one less positive valence state,
BB• refers to the B site cation increasing one valence charge and VO•• refers to the
formation of an oxygen vacancy. The Kroger-Vink notation, where the brackets indicate
concentrations of the indicated species, is utilized in this equation. The equation means
that for every substitution made into the A site, where the new cation has a valence one
less than the original cation, there must be a compensation for the charge difference
created by this substitution. The compensation can either come from an increase in the
12
valence of the B site cations (electronic compensation) or the formation of oxygen
vacancies (ionic compensation) [8]. This increase in oxygen vacancy population leads to
an increase in ionic conductivity.
Relevant Cathode Systems
LaSrMnO3
The La1-xSrxMnO3-δ (LSM) system is the most commonly used cathode material
for SOFCs. Under normal operating conditions, LSM exhibits a negligible amount of
ionic conductivity, which limits the cathode reaction to the triple-phase boundary where
the cathode, electrolyte and oxygen are all in contact [6, 7, 9-21].
The electrical
conductivity of this material is acceptable at the operating temperatures of the SOFC;
however, increasing these conductivities (electrical and ionic) would decrease the
electrode polarization and subsequently increase the fuel cell’s performance [11]. The
major setback of the LSM system is that the cathode and the yttria-stabilized zirconia
(YSZ) electrolyte form highly resistant products, such as La2Zr2O7 at high temperatures
[12]. This reaction greatly reduces the fuel cell performance and the lifetime of such a
cell.
At SOFC operating temperatures, LSM is stable in oxidizing atmospheres but
decomposes under highly reducing conditions. LSM decomposes directly to La2O3 and
MnO at critical oxygen partial pressures of about 10-14 to 10-15 atm at temperatures above
1100oC [11].
At lower temperatures from 350oC to 600oC, this cathode tends to
13
transform to other phases such as La2MnO4, La4Mn4O11, La8Mn8O23, and SrMnO3 [14].
Nonstoichiometry has an influence on the stability of LSM. Lanthanum excess can
precipitate into La2O3 formation; however, lanthanum deficiencies can lead to Mn3O4
formations. The lanthanum deficiency should not exceed 10% throughout the matrix [67].
LSM is an intrinsic p-type electrical conductor due to the formation of cation
vacancies. The electrical conductivity of LSM takes place via small polaron hopping
throughout the ceramic matrix [7]. (A polaron is defined as an electron that travels
through a solid state material that, as it passes by positive ions, attracts them and, as it
passes by negative ions, repels them. This electronic transport deforms the overall
structure slightly as electrons pass through the structure.) The electrical conductivity of
LSM increases with increasing temperature and increasing strontium concentration. The
conductivity increases from 130 S/cm to 290 S/cm at 1000oC when the strontium
concentration is increased from 10% to 50% [1].
The chemical reactions of LSM and YSZ have been extensively studied at SOFC
operating and fabricating temperatures. Above 1200oC, La2Zr2O7 is produced and a layer
5 µm thick can form at the LSM/YSZ interface if sintered at 1450oC for 48 hr [7]. With
high strontium dopant concentration (above 40%), SrZrO3 is formed, and with strontium
concentrations from 20% to 50%, La2Zr2O7 and SrZrO3 are formed at temperatures above
1400oC [6]. The formations of these phases are undesirable and detrimental to the
performance of the solid oxide fuel cell. These phases act as an insulating layer and
create thermal stresses at the interface. The thermal expansion coefficients of these
14
phases are significantly lower than that of YSZ and LSM and therefore will create
undesirable stresses at the cathode-electrolyte interface.
These stresses can cause
delamination which can lead to severe cracking within the entire fuel cell plate [1].
PrSrMnO3
The Pr1-xSrxMnO3-δ (PSM) system has been studied by many as a candidate for an
alternative cathode for the SOFC [23-28]. Praseodymium’s ion size is slightly greater
than lanthanum’s, which could have an impact on the perovskite structure. This means
that an excess of Pr could have more of impact than an excess of La on the cathodic
performance. However, at high temperatures Pr changes oxidation states from Pr+3 to
Pr+4; this should increase the electrical conductivity of the ceramic and lower the cathodic
overpotential because La consists of only one oxidation state of La+3 [22]. Therefore, the
replacement of La with Pr should increase the overall cathodic performance, which is
shown in recent research. Electrical conductivity measurements and cathodic
overpotential for the PSM system have been reported much better than the traditional
cathode material, LSM. In recent studies, Pr deficiencies in the overall structure have
been emphasized in the research [23-28].
X. Huang et al. have reported research on Pr0.6-xSr0.4MnO3 with x = 0, 0.01, 0.05,
0.1, 0.15, and 0.2 [23]. The XRD results of this system show that the main structure is
perovskite with small impurities of SrMn3O6-δ and Pr6O11. Similar to the LSM system,
The Pr6O11 phase results from an excess of Pr, when x is 0.01 and 0. The SrMn3O6-
15
δ phase
is evident as x increased and resulted from an excess of Sr and Mn ions.
Therefore, some Pr deficiency can produce a single phase perovskite structure.
The electrical conductivity of this system increased with an increase in Pr
deficiency. This seems to represent an increase in mobility and concentration of the
polarons as Pr deficiencies increased.
At 750oC, the maximum conductivity was
measured at 121.7 S/cm when x = 0.05. With the formation of SrMn3O6-δ phase, the
electrical conductivity decreased because this phase’s conductivity is about 25 times less
than that of the single phase perovskite PSM structure. The PSM set measured a higher
conductivity than a similar LSM system, which suggests replacing La with Pr increases
the electrical conductivity. The cathodic overpotential for this system was lower than the
LSM system, with Pr deficiency lowering this value, and x = 0.05 produced the lowest
cathodic overpotential [23].
H. Ullman et al. reported results for Pr0.65Sr0.3MnO3, Pr0.7Sr0.3MnO3, and
Pr0.8Sr0.2MnO3 ceramics. Using XRD analysis, it was shown that this ceramic developed
into a perovskite structure after being sintered at 1450oC for 20 hours. The thermal
expansion coefficient Pr0.65Sr0.3MnO3 was measured at 11.6 * 10-6K-1, which is close to
the values of the commonly used YSZ electrolyte and Ni-YSZ anode. The electrical
conductivities of the system were also measured. As the Sr concentration increased, the
conductivity also increased with Pr0.65Sr0.3MnO3 being the highest.
The ionic
conductivity was also measured, demonstrating that the substitution of La with Pr did not
influence oxygen permeation. Therefore, the oxygen permeation throughout this system
16
is negligible but should be further investigated because maximizing the ionic
conductivity would lead to more effective cathode performance [27].
17
CHAPTER 3
EXPERIMENTAL PROCEDURES
Glycine-Nitrate Pyrolosis
Five compositions of Pr1-xSrxMnO3-δ where x = 0.10, 0.20, 0.30 and (Pr1xSrx)0.98MnO3-δ
where x = 0.20 and 0.30 were created using a glycine-nitrate pyrolosis
process. The appropriate amounts of praseodymium, strontium and manganese nitrate
salts were mixed together in a large glass beaker to obtain the desired compositions. The
concentrations of these nitrate salts were determined using either a gravimetric or
complexiometric titration.
The gravimetric method is the simpler of the two methods, but may only be
performed on the nitrate salt concentrations if the element of interest has only onevalence state, like praseodymium (+3) and strontium (+2) at lower temperatures. For the
manganese nitrate salt, complexiometric titration was utilized to obtain the concentration.
Once the aqueous nitrate salts are mixed, glycine powder was added to the solution at
twice the stoichiometric quantity to complete the glycine-nitrate combustion reaction.
The nitrate salts and glycine are stirred together until the glycine is completely dissolved.
In the tables below, sample calculations for the mass of nitrate salt and mass of
glycine powder can be found, along with a table of all of the masses mixed in order to
obtain the correct ceramic composition. In a tall stainless steel pot, 100 mL of the
18
glycine-nitrate solution is added and placed on a hot plate inside of a fume hood, while
the remaining solution is continuously stirred. Because of the tall height of the pot and
the small amount of liquid being used, the solution does not boil over. The water in the
solution is allowed to boil away to concentrate the nitrates and glycine. Once the solution
is concentrated, the glycine reacts with the nitrates in an exothermic reaction reaching
temperatures above 1200˚C [26]. This reaction’s products include an oxide ceramic
powder in the form of ash, with byproducts of nitrogen, oxygen, water and carbon
dioxide gases, and heat. The ash is collected from the bottom of the pot and another 100
mL of solution is added to the pot to begin the process again until no solution remains.
Table 1: PSM compositions and nitrate solutions for glycine-nitrate combustion.
Compositions
Pr0.9Sr0.1MnO3-δ
PSM 10
Pr0.8Sr0.2MnO3-δ
PSM 20
Pr0.7Sr0.3MnO3-δ
PSM 30
(Pr0.8Sr0.2)0.98MnO3-δ
PSM 20 A
(Pr0.7Sr0.3)0.98MnO3-δ
PSM 30 A
Pr(NO3)3
0.457 mol/kg
1969.37 grams
Sr(NO3)2
2.0254 mol/kg
49.37 grams
Mn(NO3)2
Glycine
1.163 mol/kg
859.84 grams 390.36 grams
1750.55 grams
98.75 grams
859.84 grams 380.35 grams
1531.73 grams
148.12 grams
859.84 grams 370.35 grams
1715.53 grams
96.77 grams
859.84 grams 374.75 grams
1501.09 grams
145.16 grams
859.84 grams 364.94 grams
19
Table 2: Sample mass calculations for nitrate solution and glycine.
Sample Calculations of the mass of nitrate salts used in the
glycine-nitrate pyrolosis to create 1 mol of PSM 10
C PrNO3 := 0.457
N Pr := 0.9 mol
N Sr := 0.1 mol
N Mn := 1mol
mol
kg
C SrNO3 := 2.0254
mol
C MnNO3 := 1.163
mol
Nitrate salt concentrations were
calculated using gravimetric
or titration methods.
kg
kg
Calulation to determine mass of nitrate salts used in combustion reaction
M PrNO3 :=
M SrNO3 :=
N Pr
M PrNO3 = 1969.37 gm
C PrNO3
N Sr
M SrNO3 = 49.37 gm
C SrNO3
N Mn
M MnNO3 :=
M MnNO3 = 859.85 gm
C MnNO3
Calculation of the mass of fuel or glycine supplied to the reaction
Pr := 3
Moles of nitrates in 1 mol of
individual nitrate salt
Sr := 2
Mn := 2
N PrNO3 := N Pr ⋅ Pr
N Total_NO3
N SrNO3 := N Sr ⋅ Sr
N MnNO3 := N Mn ⋅ Mn
:= N PrNO3 + N SrNO3 + N MnNO3
N Total_NO3
= 4.9 mol
Formation of 1 mol of PSM 10 requires 3 moles of oxygen atoms,
where I mol of NO3 supplies 3 oxygen atoms
N consumed
:= N Total_NO3
− 1mol
N consumed
= 3.9 mol
According to the glycine combustion reaction, every 2 moles of glycine
reacts with 3 moles of NO3
ρ glycine := 75.04
M glycine = 195.1 gm
gm
mol
M glycine :=
2
3
N consumed ⋅ ρ glycine
Mass of glycine for stoichimetric reaction
Twice this mass of glycine was mixed to create reducing conditions for this reaction
20
The glycine-nitrate reaction is [29]:
2H2CNCH2CO2H + 3NO3 => 5H2O + 4CO2 +5/2N2
Sample Preparation
Calcination
The first step after the reaction is to sieve the powder produced through glycine
pyrolosis through a 45-µm-sieve tray, so that the particle sizes are relatively uniform
before calcination begins. The powder is carefully poured into crucibles and covered to
prevent ceramic powder contamination in the furnace. These powders were heated to
1200˚C for two hours using a heating and cooling rate of three degrees per minute. This
calcination step is intended to drive any nitrates, excess oxygen and impurities out of the
powder and induces a single-phase ceramic crystalline structure. The powder densifies to
approximately 30% its original volume and occasionally needs to be ground back down
to powder after calcination using mortar and pestle.
Attrition Milling
The calcined powder is first sieved through the 45-µm-sieve tray and is then
weighed. Isopropanol is measured to half the mass of the ceramic powder. In the
attrition-milling canister, half of the alumina beads being used are added, then the
ceramic powder is added, next the isopropanol, and finally the rest of the alumina beads.
This canister is attached to the attrition-milling machine and left on for two hours. The
21
purpose of this step is to grind the particulate powder to a size under a micron. This is
essential for the particles to adhere well to the YSZ electrolyte for half-cell testing. After
attrition milling, a small sample is analyzed in a particle size analyzer to ensure the
particle size is under a micron and is relatively uniform.
Ink Preparation
For half-cell testing, an YSZ electrolyte pellet is screen printed with cathodic ink.
This ink is prepared by measuring 10 grams of the calcined powders and mixing it with
5.38 grams of screen print binder Ferro binder B-75717. This binder consists of a
polymeric material, polyvinyl buytral, with a carbitol acetate solvent.
This binder
completely decomposes at 350oC in an air atmosphere with adequate airflow. The weight
percent of powder to binder gives a 65% solids loading in the prepared ink. Once the
powder and binder are thoroughly mixed together, the mixture is added to a three-roll
mill (Exakt 11671 three-roll mill) and rolled through twice. The three-roll mill is used to
thoroughly mix the powder and binder together so that each ceramic particle is
thoroughly coated with the screen print binder. The ink is then put into jars and labeled
accordingly.
Pellet and Bar Pressing
Some of the calcined powder is pressed into rectangular bars 4.5 cm in length and
1.6 cm wide for electrical conductivity, Seebeck, and dilatometry measurements. Some
of the calcined powder can also be pressed into circular pellets of a diameter of 3.2 cm
22
for oxygen permeation measurements. For a rectangular bar, 7 grams of powder are
weighed out and evenly distributed throughout the dye and pressed with the top part of
the dye, using uniaxial pressure of about 6 MPa, followed by cold isostatic pressing
above 500 MPa. For the circular pellet, 5 grams of powder are measured and again
evenly distributed throughout the dye and gently pressed to the top of the dye. It is
pressed using uniaxial pressure of about 2 MPa, followed by cold isostatic pressing above
500 MPa. These bars and pellets are then sintered to densify and add tensile strength to
the piece before testing.
XRD Evaluation
Phase Purity
Phase purity was determined by x-ray diffraction (XRD) analysis using Cu Kα
radiation (XRG 3100, Philips Electronic Instrument, Mahwah, NJ). The spectra obtained
were compared to known spectra of similar perovskite compounds to determine phase
concentration after background or noise removal using Jade+ v2.1 software (Materials
Data Inc., Livermore, CA). The theoretical densities were calculated using the lattice
parameters obtained from diffraction analysis.
These theoretical densities can be
compared to the bulk densities measured by the Archimedes method to determine if the
samples are dense enough for oxygen permeation experiments. By comparing the bulk
density to the theoretical density it is possible to determine the amount of open porosity
in a sample.
23
Archimedes Density
The Archimedes method was used for finding the apparent density of the sintered
samples. The Archimedes Buoyancy Principle states that when an object is immersed in
a liquid it will be lighter by an amount equal to the mass of the liquid that the object
displaces. The density can then be calculated by collecting the dry, suspended, and wet
weights of the sintered samples. The suspended and wet weights were obtained by
submerging the samples in ethanol and then placing in a vacuum chamber until all the
open pores of the sample had been infiltrated with the ethanol. The samples were then
weighed as they were suspended completely immersed in a beaker of ethanol to obtain
the suspended weight. By drying the sample and immediately weighing it, the wet
weight was obtained before the ethanol could evaporate from the open pores, allowing a
measurement of the bulk density of the samples to be calculated.
Dilatometry
The coefficient of thermal expansion for the compositions shown in Table 1 was
determined by dilatometric analysis (Unitherm Model 1161, Anter Laboratories, Inc.,
PA). Linear thermal expansion was conducted on bars (~1/6”x1/6”x1”) at a ramp rate of
2oC/min in air. All dimensions were measured before the dilatometry. Data points were
taken as the temperature increased and then decreased. As the temperature decreases, the
slope of the line of the strain vs. temperature is calculated for thermal expansion
coefficient values.
24
Electronic Conductivity
Electrical conductivity for the five compositions consisting of a single phase was
measured using a four-point AC conductivity method. Platinum electrodes were attached
as shown in figure 3.1.
Platinum leads
Space between
leads ~1.4 cm
2.5 cm
0.3 cm
0.3 cm
Figure 3.1: Sample used for the four-point AC conductivity experiments.
The samples were cut to the dimensions ~2.5 cm x 0.3 cm x 0.3 cm and notched
with a diamond saw where the platinum wraps were placed around the sample. Platinum
paint was used to ensure the contact between the sample and the platinum electrodes.
The paint was applied prior to the wires being wrapped and twisted on the samples and
then cured at 600oC. The short leads that were wrapped around the samples were then
welded to long leads for obtaining experimental data. The sample was then placed in a
tube furnace with the leads connected to the current source and electrometer.
25
Ionic Conductivity
The amount of ionic conductivity was found by placing a 0.72-inch diameter
sample in the setup shown in figure 3.2.
Source gas in
Alumina Tube
Gold Gaskets
Sample
Zirconia EMF Sensor
nitrogen carrier plus
permeate out
nitrogen carrier in
Figure 3.2: Oxygen permeation assembly.
After the thickness was measured, the sample was sandwiched between two
alumina tubes with gold o-rings used to seal the sample to the tubes. The gold o-rings
were super glued to the alumina tubes and the sample was glued to one of the tubes.
Gravity and applied pressure provides an airtight seal from the alumina tube to gold and
gold to sample interfaces. Therefore, the only gas that would cross from top to bottom
would have to permeate through the sample. An outer alumina tube (not shown in figure
26
3.2) is used to provide stability to the structure and another interface seal to the gold. The
furnace was ramped up to 950oC to allow the gold to liquefy sufficiently to form a seal
but not ooze down the side. The furnace was then cycled from 950oC to 200oC at
2oC/min. Atmospheric air (20.98% oxygen) was flowed over the upper side of the
sample at a rate of 100 cc/min. The lower side had nitrogen flowing at a rate of 25
cc/min. This created an oxygen gradient from one side of the sample to the other. The
exhaust from the lower side was piped to a zirconia EMF oxygen sensor. The voltage
measured from the sensor is a measure of the oxygen flux through the sample.
Seebeck Measurements
In figure 3.3, a diagram of the assembly of the Seebeck coefficient measurement
is shown.
Figure 3.3: Assembly structure for Seebeck coefficient measurements.
On one end of a ceramic test bar, a heating element is used to create a temperature
gradient across the sample with thermocouples on each end to measure the temperature
gradient. Two voltage taps are placed on each end of the bar to measure the voltage drop
27
across the sample due to the applied temperature gradient. The entire sample is heated
and cooled from 200oC to 900oC. At each 50oC interval measured on thermocouple 2,
the temperature at thermocouple 1 was measured and used to calculate the temperature
gradient between the two thermocouples. As the sample was heated from 200oC to
900oC, then cooled back to 200oC, the temperature difference ranged from -20oC to 30oC
approximately fifteen data points are taken throughout this temperature gradient in order
to allow an accurate line to be plotted through these points of voltage drop vs. the
temperature gradient. The slope of the line of the voltage drop vs. the temperature
gradient is the measured Seebeck coefficient.
Half – Cell Measurements
A diagram of the assembly of the half-cell measurement is shown in figure 3.4.
Figure 3.4: Half-cell measurement set-up.
28
Electrodes are screen-printed on yttria-stabilized zirconia (DKKK 8YSZ) pellets
with 8 molar% yttria. These pellets have been uniaxially pressed at 6 MPa and then cold
isostatic pressed at 500 MPa. The electrolyte pellet is 12.5 mm in diameter and 4 mm
thick. A probe cavity is drilled to about 1 mm from the working electrode side.
After the electrolyte pellet is screen-printed with platinum on the side with the
small hole and the opposite side has a cathode layer, the half-cell pellet is placed in
between two platinum screens. A three-electrode cell configuration is used as illustrated
in figure 3.4. A three electrode cell uses a working electrode, a counter electrode and a
reference electrode to make the half cell measurement. A Lugin-Haber type reference
electrode was used in the assembly [30]. A 0.5 mm platinum wire with a 0.75 mm silver
bead on the tip is pressed into the hole in the sample. This wire is used as a reference
point to minimize the resistance through the electrolyte. Alumina plungers are affixed to
an alumina tube using spring tension and are used to provide good contacts for the
platinum screens and cathode and platinum layers on the half-cell pellet. The working
electrode is the cathode side while the counter electrode is the platinum side of the halfcell. By connecting this assembly to a Solartron SI 1287 potentiolstat/galvanostat, halfcell potential is measured through the use of cyclic voltamograms with current interrupt
embedded in the software program. The applied current ranged from –2A to 2A with the
voltage drop ranging from –0.5V to 0.5V, which limited the current range with a scan
rate of 10mV/sec. This current vs. voltage curve can be modeled using a hyperbolic sine
curve to determine the resistance in the cathode and the current exchange density of the
cathode-electrolyte interface.
29
CHAPTER 4
RESULTS AND DISCUSSION
XRD Evaluation
Phase Purity Peaks
Figure 4.1 shows XRD phase peaks for the entire PSM data set after calcination at
1400oC for an hour. A silicon powder was used as a reference to allow aligning the phase
peaks if there is offset among the data. The XRD peaks in figure 4.1 from the top
progress through the sample from PSM 10, 20, to 30 and then the A site deficient
ceramics with PSM 20 A to PSM 30 A.
30
Figure 4.1: XRD phase peaks for the PSM data set with references for silicon, PSM and
Hausmannite.
The different phase peaks of the sample set show that each sample develops into a
single perovskite phase, however a slight peak showing a slight excess in manganese is
detectable, which develops a hausmannite phase, Mn3O4. XRD peaks show phases in
ceramic with at least a five percent phase concentration throughout the structure; and thus
throughout these ceramics, five percent of their structure contains this hausmannite
phase.
As the strontium concentration increases, the excess of manganese is more
prevalent with slightly stronger peaks. The A site deficient ceramics contained slightly
31
stronger peaks overall than its stoichiometric partner, and even PSM 20 A has more
manganese in the hausmannite phase than PSM 30. This phase may disappear with an
increased sintering temperature or a longer sintering time or both.
Relative Density
From the lattice parameters that are calculated from the shifts and width of the
phase peaks from X-ray diffraction, the theoretical density, which is a calculation of the
density of the ceramic material without porosity, can be calculated.
Through the
Archimedes density approach discussed earlier, the actual density of a ceramic bar can be
calculated and then compared with the theoretical density to determine the percent
density. In table 3, calculations of the bulk density and percent density, which is the bulk
density/theoretical density, of the sample set can be found.
Table 3: Relative and percent densities calculations
Ceramic
PSM 10
PSM 20
PSM 20 A
PSM 30
PSM 30 A
Dry Mass
(g)
9.793
8.952
7.559
7.614
14.542
Suspended
Mass (g)
8.561
7.824
6.593
6.64
12.688
Saturated
Mass (g)
9.808
8.956
7.573
7.624
14.544
Theoretical
Density
6.5594
6.5844
6.6021
6.6207
6.6865
Bulk
Density
6.17
6.21
6.06
6.08
6.12
Percent
Density
94.1
94.4
91.8
91.8
91.6
32
The equation used to find the bulk density of the material is as follows:
ρ bulk
ρ ethanol ⋅ mdry
msat − msups
where mdry, msat, and msusp ate the dry mass, saturated mass and suspended mass
respectively.
These relative densities need to be about 95% dense and therefore each sample
was sintered at 1500oC for 2 hours at a ramp rate of 2oC/min. After this sintering, the
ceramic bars and pellets would be dense enough to properly measure the oxygen
permeation, electrical conductivity, and Seebeck coefficient.
Dilatometry
Sintering Study
After calcination at 1200oC for 2 hours a sintering study was performed to
determine the temperature at which the ceramic densifies and the temperature to which an
ink preparation would expect to adhere to an electrolyte pellet for half-cell testing. This
data is shown in figure 4.2.
33
0.02
0.01
Strain (∆L/Lo)
0
-0.01
-0.02
PSM 10
-0.03
PSM 20
-0.04
PSM 20 A
-0.05
PSM 30
PSM 30 A
-0.06
0
200
400
600
800
1000
1200
1400
1600
o
Temperature ( C)
Figure 4.2: Densification Study of samples up to 1400oC.
TEC Calculation
The thermal expansion coefficient was determined using the data from the
dilatometer. After the sintering study, data of strain vs. temperature as the temperature
decreased was taken. The slope of this line through the temperature range of 200oC to
1400oC was calculated for the thermal expansion coefficient and is shown in figure 4.3.
The thermal expansion coefficients for a common electrolyte (8YSZ) and anodic material
(NiO-YSZ) are also displayed on this graph in order to compare the sample set with
commonly used solid oxide fuel cell material.
34
14.00
TEC (∆T/∆L/Lo) (10^-6)
13.00
12.00
11.00
Stoichiometric
10.00
A site deficient
8 YSZ
50% NiO YSZ
9.00
10%
20%
30%
Strontium Fraction in Perovskite Structure
Figure 4.3: TEC measurements of sample set with comparison to common electrolyte and
anode material.
Analysis
In the sintering study, the graph in figure 4.2 should eventually level off to display
the maximum density observed by the ceramic material; however, due to limitations of
the experimental setup, a full range of temperatures was not able to be completed. A
more useful calculation from this data is an expected sintering temperature for adhesion
to the YSZ electrolyte material. This will occur near the “knee” of the graph or at the
point where the ceramic starts to densify. The temperature that was tested successfully
for this adhesion was 1150oC. Also apparent in the sintering curve is the trend in
35
densification as the strontium concentration is increased. As strontium concentration
increased so did the temperature at which full densification occurred. By creating an A
site deficiency in the matrix, the densification temperature is also increased. PSM has
very refractory material properties, which contributes to high sintering temperature
throughout the sample set.
The strain vs. temperature line that was used to determine the thermal expansion
coefficient (TEC) was linear throughout the temperature range, which means that the
sample’s structure was very stable. As the strontium concentration increases, the TEC
value also increases. The A site deficient set follows the same trend and is within the
margin of error of the corresponding stoichiometry set. These coefficients are also
compared with commonly used solid oxide fuel cell materials in figure 4.3. 8YSZ is
right in the middle of the sample set with PSM 20 having the same coefficient. The
anode material Ni-YSZ is at the high end of the TEC coefficient but at the same level as
PSM 30. Therefore, the ceramic materials tested in the sample set can all be used with
Ni-YSZ except PSM 10 because the coefficients differ by more than 3*10-6 [1].
Electronic Conductivity
Calculations
Electrical conductivity data are shown in the figure 4.4 for the complete data set
for the temperature range from 200oC to 950oC using a four point AC testing method as
discussed earlier.
36
300
Conductivity (S/cm)
250
200
150
100
50
0
100
200
300
400
500
600
PSM 30
PSM 30 A
PSM 20 A
PSM 20
PSM 10
LSF 20
700
800
900
1000
Temperature (oC)
Figure 4.4: Electrical conductivity measurement from 200oC to 950oC.
The conductivity values presented in figure 4.4 are for the bulk electrical
conductivities of the samples. Since the ionic conductivity is less than 1% of this bulk
conductivity, the values are regarded as dominantly electronic.
The single phase
compositions tested (except for PSM 30) exhibited an increase in electrical conductivity
with increasing temperature. This behavior is typical for small polaron conductors where
the electronic conductivity of the material is dependant on the mobility of thermally
activated localized charges.
All of the compositions had a temperature where their conductivity leveled off
and then decreased or stayed constant. For example, the electrical conductivity for PSM
20 increased with increasing temperature until it reached about 600oC, where it leveled
off or increased only slightly. This is most likely due to a saturated state of electrons in
the conducting band.
37
An Arrenhius plot is constructed in figure 4.5 where the natural log of the
electrical conductivity multiplied by the temperature is graphed versus the inverse
temperature. The activation energies can be determined from the slopes of these curves
and are plotted in figure 4.6 for comparison.
13
ln (ST) (KS/cm)
12
11
PSM 30
PSM 30
A
PSM 20
A
PSM 20
10
9
0.5
1
1.5
1000/T (K)
Figure 4.5: Arrenhius plot of electrical conductivity measurement.
2
2.5
38
Activation Energy (eV)
0.2
0.15
0.1
0.05
Stoichiometric
98% A site
0
0
10
20
30
Percent Strontium
Figure 4.6: Activation energies for electrical conductivity.
Analysis
The electrical conductivity is an important factor in determining the effectiveness
of a cathode material. Typically a conductivity value of 100 S/cm in the temperature
range of 600oC to 800oC is preferable [8]. The sample set, except for PSM 10, all
reached this value and in fact doubled and almost tripled this value. PSM 10 barely
reached 100 S/cm at 800oC.
As the strontium concentration increased, the activation
energy to create conductance decreased. The activation energy is the necessary energy to
raise electrons to the conduction band. Therefore, the activation energy is an inverse
function of the total conductance throughout this sample set. Lower activation energy of
electrical conductivity translates to a raise in the ease of conductance and therefore a
higher conductivity level can ensue.
A comparison of the PSM sample set with a commonly used cathodic material set,
lanthanum strontium ferrite (LSF) is shown in figure 4.4. The PSM sample set, except
39
for PSM 10, has a significantly higher electrical conductivity than that of LSF 20, which
should translate into a higher cathode effectiveness in the solid oxide fuel cell.
Ionic Conductivity
Calculations
The ionic conductivity was determined by measuring the flux of oxygen that
permeated through a sample of known dimensions. The following equation was used to
determine the ionic conductivity [1].
σ=
4 FJt
⎡ Po 1 ⎤
RT ln ⎢ 22 ⎥
⎣ Po 2 ⎦
where F is Faraday’s constant, J is the oxygen flux, t is the sample thickness, K is the
Boltzman constant, T is the absolute temperature, Po 12
and Po 22 are the oxygen partial
pressures above and below the sample. The use of this equation requires the assumption
that the oxygen flux is dominated by the bulk ionic conductivity and not the surface
kinetics.
In figure 4.7 oxygen permeation data is shown for the sample set for
temperatures of 200oC to 950oC.
40
Ionic Conductivity (S/cm)
0.25
0.2
0.15
PSM 20
PSM 30 A
PSM 30
PSM 10
PSM 20 A
0.1
0.05
0
200
300
400
500
600
700
800
900
1000
o
Temperature ( C)
Figure 4.7: Oxygen permeation from 200oC to 950oC.
Analysis
The oxygen permeation for PSM 20 behaved as initially expected through
research of similar ceramics.
In this sample, the oxygen flux through the sample
increases as the temperature increases. This correlates to a thermally activated response
to ionic conductivity. Each sample was tested through the temperature regime at least
three times to improve data accuracy, and each data set, including PSM 20, had the same
conductivity through this temperature range for each temperature sweep. The oxygen
permeation data for the rest of the series shows little to no ionic conductivity through the
temperature range of 600oC to 950oC. At lower temperatures, the oxygen permeation
41
slightly increases as the temperature decreases. The major conclusion to draw from this
data is that the ionic conductivity for much of the series is negligible through the
temperature range of a typical operating solid oxide fuel cell except for PSM 20.
Seebeck Measurements
Calculations
The Seebeck coefficient is displayed through the temperature range of 100oC to
950oC in figure 4.8. This coefficient is a measurement of a voltage drop created as a
Seebeck Coefficient (∆µ V/∆Τ ) (10^-6)
result of a temperature gradient across a ceramic bar.
20
0
PSM 30 A
PSM 30
PSM 20 A
PSM 20
PSM 10
-20
-40
-60
-80
-100
0
100
200
300
400
500
600
700
800
Temperature (°C)
Figure 4.8: Seebeck measurements for the sample set from 100oC to 950oC.
900
1000
42
Analysis
The law of Magnus states that for a material that is homogenous and isotropic, the
Seebeck EMF is independent of the temperature distribution within the material and
depends only on the temperature at the junctions.
The Seebeck EMF satisfies the
following equation [33]:
(
)
Vab T1 , T2
(
)
(
)
Vab T1 , Tc + Vab Tc , T2
where T1, T2, and Tc are arbitrary temperatures.
The Seebeck coefficient is defined by the following equation [33]:
( )
α ab T1
lim
T2 → T1
(
)
Vab T1 , T2
T2 − T1
where αab is the Seebeck coefficient. Note that the Seebeck coefficient is not dependent
on some arbitrary Tc temperature but only T1 and T2. To apply this equation, one side of
the bar had a fixed temperature and the opposite side’s temperature was varied to create
the temperature gradient. The slope of the line of voltage drop versus temperature
gradient is calculated when the temperature gradient passes through zero.
The Seebeck coefficient should increase in magnitude with an increased
temperature if the electrical conductivity increases with temperature and a simple
mechanism of conductance exists within the structure of the ceramic. PSM 10 shows this
dependence on temperature. For a true small polaron conductor, an increase in Seebeck
coefficient is expected as the strontium concentration increases within the matrix because
the electrical conductivity and the charge carrier concentration increase. The Seebeck
43
coefficient should increase as well.
However, this behavior did not always occur.
Between PSM 10 and 20, the electron conduction became more complicated. In PSM 10,
the electrons mainly traveled from the high temperature side to the cooler temperature,
while the rest of the PSM series performed the opposite dominant traveling. An n-type
conductor has a negative Seebeck coefficient and a p-type conductor has a positive
Seebeck coefficient. Therefore between PSM 10 and 20, the ceramic structure changed
conductor types from n to p. Considering the ionic conductivity of the series was
negligible, except for PSM 20, a true electrical conductance can be observed. PSM 20
exhibited a balance between n and p type conduction and as the strontium concentration
increased the Seebeck coefficient increased as well.
Half – Cell Measurements
Calculations
Half cell measurements are shown with current versus the cathode potential in
figure 4.9.
These measurements were performed using a Solartron SI 1287
potentiolstat/galvanostat. Cyclic voltamograms using a current interrupt technique were
utilized for this measurement.
44
1
Current (A/cm2)
0.8
0.6
PSM 30
PSM 20
0.4
PSM 10
0.2
0
0
0.1
0.2
0.3
0.4
0.5
Cathode Potenial (V)
Figure 4.9: Half cell measurement for sample set at 850oC in air.
PSM 10 data at 850oC with air and pure oxygen on the cathode side are shown
with a hyperbolic sine curve in order to model the area specific resistance and the overall
chemical reaction constant in figure 4.10.
45
1.2
1
sinh fit
Air Data
Current (A/cm²)
0.8
Oxygen Data
sinh fit
0.6
0.4
0.2
0
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
0.5
Cathode Potential (V)
Figure 4.10: Example of hyperbolic sine curve fit to PSM 10 data at 850oC.
In the table below, the entire PSM series from 700oC to 850oC was modeled with
a hyperbolic sine curve in order to compute electrocatalytic activity.
46
Table 4: Tabulated values of chemical reaction constants and area specific resistance
throughout the cathode layer.
Ceramic
PSM
10
PSM
20
PSM
20 A
PSM
30
PSM
30 A
Io
RASR
Io
RASR
Io
RASR
Io
RASR
Io
RASR
850oC
Oxygen
Air
0.02205 0.0398
1.6036 3.8294
0.055
0.0227
1.4536
3.468
0.0859 0.0299
1.326
3.152
0.0526 0.0142
1.409
4.179
0.0874 0.0327
1.256
3.074
800oC
Oxygen
Air
0.0252 0.0022
3.4823 23.645
0.0404 0.0045
2.4613 14.269
0.0141 0.0032
5.4933 20.231
0.0221 0.0066
3.341
9.887
0.0407 0.0067
5.685
11.422
750oC
Oxygen
Air
0.0026 0.00074
24.246
85.899
0.0029 0.00107
22.29
58.956
0.00183 0.00103
32.642
61.339
0.0043
0.0023
15.022
27.966
0.0036 0.00148
18.119
42.907
700oC
Oxygen
Air
0.00022 0.00007
275.39
889.57
0.00045 0.00031
141.227 204.65
0.00046 0.00034
135.81
185.26
0.00107 0.0008
59.289
79.566
0.00078 0.00053
80.61
119.95
*Note: Io is in A/cm2 and RASR is in Ω/cm2
The entire series of cathodes pictured in figures 4.11 to 4.15 were sintered on
individual YSZ electrolytes at 1150oC for 2 hours. The scanning electron microscope
picture of the half cell of PSM 10 after the cathodic overpotential was measured is shown
in figure 4.11.
The porous cathode layer pictured in figure 4.11 is about 3 µm thick and
is well adhered to the dense YSZ electrolyte. Energy Dispersive Spectrometer (EDS)
measurements were used to identify the molar percentage of different elements in the
cathode structure.
The darker regions contained more manganese while the lighter
regions contained more praseodymium.
By scanning the entire region, the molar
concentration of praseodymium was approximately 90 % of the molar concentration of
manganese and the molar concentration of strontium was approximately 10 % of the
molar concentration of
manganese. Also, scanning the YSZ electrolyte, migration of
praseodymium, strontium, or manganese was not discovered. This suggests that there
were no adverse reactions with the cathode layer of PSM and the YSZ electrolyte. This
47
would eliminate the barrier layer between the cathode layer and the electrolyte that is
currently being employed. This is very beneficial because it eliminates one processing
step and therefore reduces production cost of the fuel cell plate.
Figure 4.11: PSM 10 half cell after testing.
48
The scanning electron microscope picture of the half cell of PSM 20 after the
cathodic overpotential was measured is shown in figure 4.12.
Figure 4.12: PSM 20 half cell after testing.
49
The scanning electron microscope picture of the half cell of PSM 20 A after the
cathodic overpotential was measured is shown in figure 4.13.
Figure 4.13: PSM 20A half cell after testing.
50
The scanning electron microscope picture of the half cell of PSM 30 after the
cathodic overpotential was measured is shown in figure 4.14.
Figure 4.14: PSM 30 half cell after testing.
51
The scanning electron microscope (SEM) picture of the half cell of PSM 30 A
after the cathodic overpotential was measured is shown in figure 4.15.
Figure 4.15: PSM 30A half cell after testing.
Some trends can be interpreted from the series of SEM pictures. As the strontium
concentration increases, the porosity of the cathode layer also increases and the A site
deficiencies have more porosity than their stoichiometric partner with PSM 20 A having
higher porosity than even PSM 30. As this porosity increases, the thickness of the
cathode layer also increases. PSM 30 A’s cathode layer thickness is about 12 µm while
PSM 10’s is about 3 µm. Each ceramic in this series adhered well to the YSZ electrolyte
52
after sintering at 1150oC for 2 hours. Considering the oxygen permeation is negligible
for the PSM series except PSM 20, porosity in the cathode layer is a very important
parameter in order to have enough oxygen flux to the triple phase boundary to increase
the reduction reaction.
This parameter and the electrical conductivity of the series
correlates well with the cathodic overpotential measurements, meaning as the porosity
and electrical conductivity increase, the cathodic overpotential is lower.
Analysis
These half cell measurements show the electrocatalytic activity of the cathode
itself. The chemical reaction on this side is as follows:
O2(gas) Æ O(adatom) + 2e- Æ O2-(in the electrolyte)
A hyperbolic sine curve is used to model these curves to better interpret the
graphs. Through the use of this equation, the chemical reaction constant of the equation
above and the area specific resistance can be computed. This equation is as follows:
α c⋅ F ⎞
⎛⎜ α a⋅ F
⎜ R⋅ T + e R⋅ T
⎛ α ⋅ F⋅ η ⎞
I Io⋅ ⎝ e
⎠ 2⋅ Io⋅ sinh ⎜
⎝ R⋅ T ⎠
where I is the current, F is the Faraday’s constant, R is the ideal gas constant, T is the
temperature, η is the voltage.
1
I
RASR
η
⎛ α⋅F ⎞
2Io ⋅ ⎜
R⋅ T
⎝
⎠
where RASR is the area specific resistance.
53
By looking at Table 4, trends in the PSM series can be observed.
As the
strontium concentration increases, the area specific resistance decreases and the chemical
reaction constant increases. For the entire series, temperature dependence is observed; as
temperature decreases, the electrocatalytic performance of the cathode significantly
decreases, especially at 700oC.
54
CHAPTER 5
CONCLUSIONS AND RECOMMENDATIONS
The PSM series was characterized through the use of a variety of experimental
methods. XRD was used to interpret the phases in the series to determine if a single
phase perovskite structure could be made after calcination of the ceramic at 1400oC for
two hours. A sintering study was additionally performed to determine the temperature of
full densification and an effective sintering temperature to adhere to the YSZ electrolyte.
Densification happens at 1500oC, while the cathode ink was sintered on the electrolyte at
1150oC.
The electrical conductivity also was measured using a standard four probe AC
measurement technique. These conductivity measurements showed a higher conductivity
than the traditional LSM cathode material. An upper limit on the conductivity seemed to
be above 30% strontium concentration; therefore, more research should be performed
with strontium concentrations above 30% until this upper limit can be determined. The
activation energies for these conductivities were also calculated using an Arrenhius plot,
with these activation energies decreasing as the strontium concentration increased.
The oxygen permeation of this series was measured using an oxygen transport
method. Except for PSM 20, the oxygen conductivity was negligible for the series. More
research should be undertaken in order to increase the oxygen flux through the sample
and to determine the mechanism of transport through PSM 20. SEM pictures of the used
55
pellets can be used to determine densification and find any cracks in the pellets. The
addition of another multivalent dopant on the B site may increase the oxygen permeation.
Another measurement was the Seebeck coefficient, which determined that the
electrical conduction of the ceramic changed from an n type conductor to a p type
conductor as the strontium concentration increased. More research should be performed
to better understand this phenomenon with PSM 5 and PSM 15 being a good start to this
further research. Thermogravimetric analysis should be used to determine the charge
carrier concentrations for the data set.
The cathodic overpotential was measured through the use of cyclic voltamograms
using a current interrupt technique. The cathodic overpotential lowered as the strontium
concentration increased.
This correlates well with the electrical conductivity
measurements. Calcination at 1200oC does not produce a single phase structure for these
materials. Therefore, the ceramic powders should be calcined at 1400oC instead; and
then more inks should be prepared and tested. These results could be compared with the
results from this study to determine the importance of having a single phase perovskite
structure.
56
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